STAR Flow, Chirality and Vorticity PWG

[subhash <subhash AT rcf.rhic.bnl.gov>]

Dear Shuai,

It seems like some of the suggestions are not incorporated in this 
version. Is this the correct version to look for?Could you correct the 
typos and fix the missing X/Y axis labels as suggested?

Thanks and regards,
Subhash

On 2022-11-27 05:06 PM, zs155167 wrote:
> Dear Subhash,
>
>   Thank s for your comments and suggestions!
>   I have updated my slide for CPOD2022 here:
> https://drupal.star.bnl.gov/STAR/system/files/CPOD2022_Shuai_Zhou_1.pdf
>   Thank you very much!
>
> Best and regards,
> Shuai Zhou
>
> ------------------ Original ------------------
>
> From:  "subhash"<subhash AT rcf.rhic.bnl.gov>;
> Date:  Sun, Nov 27, 2022 11:49 AM
> To:  "周帅"<zs155167 AT mails.ccnu.edu.cn>;
> Cc:  "STAR Flow,Chirality and"<star-fcv-l AT lists.bnl.gov>;
> Subject:  Re: [Star-fcv-l] STAR presentation by Shuai Zhou for CPOD
> 2022 submitted for review
>
> Dear Shuai,
>
> Thanks for incorporating my suggestions. I have a few additional ones:
>
> General: Please check X/Y-axis labels is hidden behind figures/frames
> It would be good if X/Y axis label sizes are increased.
> In several places, 14.6 GeV instead of 14.6GeV
>
> s3: pressure gradient and interaction among ... FINAL ...
> Please add reference to flow papers
>
> s5: Sub-event method
> You could mention event plane is a proxy for reaction plane
>
> s6: left plot title: TPC Event plane
> right plot:  remove ZS in legend
> second bullet: v_2
>
> s7: Add a reference to STAR papers, where such rotations are applied
>
> s9: protons are identified ... up to pt 3.2 GeV/c
> Remove the statistical boxes inside figures.
>
> s12 & 13: Instead of squeezing two plots, you can probably animate
> them
> one by one with a larger size of figure.
>
> In one of the v2 slide, or in summary you can probably mention the
> reduction of errors in BES-II compared to BES-I.
>
> I sign off once these are addressed.
>
> Thanks and regards,
> Subhash
>
> On 2022-11-26 03:59 PM, zs155167 wrote:
> > Dear conveners,
> >
> >    I have updated my slide for CPOD2022. Please have a look at the
> new
> > version here:
> https://drupal.star.bnl.gov/STAR/system/files/CPOD2022_Shuai_Zhou_1.pdf
> >    If you have any comments and suggestions, please let me know.
> Thank
> > you very much!
> >
> > Best and regards,
> > Shuai Zhou
> >
> > ------------------ Original ------------------
> >
> > From:  "周帅"<zs155167 AT mails.ccnu.edu.cn>;
> > Date:  Wed, Nov 23, 2022 09:00 PM
> > To:  "subhash"<subhash AT rcf.rhic.bnl.gov>; "STAR Flow,Chirality
> > and"<star-fcv-l AT lists.bnl.gov>;
> >
> > Subject:  Re: [Star-fcv-l] STAR presentation by Shuai Zhou for CPOD
> > 2022 submitted for review
> >
> >  Dear Subhash,
> >
> >  Thanks for your comments and suggestion. Here are my illustrations:
> >
> > For the new BES-II 14.6 GeV pi, K, p v2 data, do you have a
> comparison
> > with BES-I that we can take a look?
> >
> >  Yes, please find my slide here:
> > https://drupal.star.bnl.gov/STAR/system/files/v2ratio.pdf [1]
> >
> > I see, you have presented individual pi, K, p v2 at FCV, but I feel
> > that
> > the NCQ scaling results especially on slide 12 and 13 are new. Could
> > you
> > discuss it today at the FCV?
> >
> > OK, I will illustrate it today at the FCV
> >
> > Do you observe any centrality dependence in NCQ scaling behavior?
> >
> > Within errors, no obvious centrality dependence is observed.
> >
> > Is it possible to make a single NCQ scaling plot, including all
> > particles measured. I mean pi, K, p (from you) and multi-stranges
> from
> > Prabhupada.
> >
> >   OK, I will contact Prabhupada about this.
> >
> >  There was some discussions at the FCV related to the
> > asymmetricmass-square selection. Could you indicate if you have done
> > any check?
> >
> > Yes, I have checkd it, please find:
> https://drupal.star.bnl.gov/STAR/system/files/star_prelimilary_update.pdf
> > [2]
> >
> > Please include, collision system, energy, TPC+iTPC etc within the
> > figure
> > where these informations are missing; Add X and Y-axis labels etc.
> >
> > s4: last bullet: identification using m2
> >
> > s6: For resolution plot, it would be good to comparison with BES-I
> >
> > s10, 11: Could you increase legends size
> >
> > Yes, I will improve it
> >
> > ------------------ Original ------------------
> >
> > From:  "subhash"<subhash AT rcf.rhic.bnl.gov>;
> > Date:  Wed, Nov 23, 2022 05:43 PM
> > To:  "周帅"<zs155167 AT mails.ccnu.edu.cn>; "STAR Flow,Chirality
> > and"<star-fcv-l AT lists.bnl.gov>;
> >
> > Subject:  Re: [Star-fcv-l] STAR presentation by Shuai Zhou for CPOD
> > 2022 submitted for review
> >
> > Dear Shuai,
> >
> > Thanks for reminder. I have a few comments and suggestions.
> >
> > General:
> > For the new BES-II 14.6 GeV pi, K, p v2 data, do you have a
> comparison
> > with BES-I that we can take a look?
> >
> > I see, you have presented individual pi, K, p v2 at FCV, but I feel
> > that
> > the NCQ scaling results especially on slide 12 and 13 are new. Could
> > you
> > discuss it today at the FCV?
> >
> > Do you observe any centrality dependence in NCQ scaling behavior?
> >
> > Is it possible to make a single NCQ scaling plot, including all
> > particles measured. I mean pi, K, p (from you) and multi-stranges
> from
> > Prabhupada.
> >
> > There was some discussions at the FCV related to the asymmetric
> > mass-square selection. Could you indicate if you have done any
> check?
> > Please include, collision system, energy, TPC+iTPC etc within the
> > figure
> > where these informations are missing; Add X and Y-axis labels etc.
> >
> > s4: last bullet: identification using m2
> >
> > s6: For resolution plot, it would be good to comparison with BES-I
> >
> > s10, 11: Could you increase legends size
> >
> > Thanks and regards,
> > Subhash
> >
> > On 2022-11-23 02:11 PM, zs155167 via Star-fcv-l wrote:
> > > Dear convenors,
> > >
> > >  I have submitted my slides for CPOD 2022. If you have any
> > suggestion
> > > or comments, please let me know. Thank you!
> > >
> > > Best regards,
> > > Shuai Zhou
> > >
> > > ------------------ Original ------------------
> > >
> > > From:  "STAR Flow,Chirality and"<star-fcv-l AT lists.bnl.gov>;
> > > Date:  Mon, Nov 21, 2022 04:18 PM
> > > To:  "STAR Flow,Chirality and"<star-fcv-l AT lists.bnl.gov>;
> > >
> > > Subject:  [Star-fcv-l] STAR presentation by Shuai Zhou for CPOD
> 2022
> > > submitted for review
> > >
> > > Dear star-fcv-l AT lists.bnl.gov members,
> > >
> > > Shuai Zhou (zs155167 AT mails.ccnu.edu.cn) has submitted a material
> for
> > a
> > > review, please have a look:
> > > https://drupal.star.bnl.gov/STAR/node/61798
> > >
> > > Deadline: 2022-11-28
> > > ---
> > > If you have any problems with the review process, please contact
> > > webmaster AT www.star.bnl.gov
> > > _______________________________________________
> > > Star-fcv-l mailing list
> > > Star-fcv-l AT lists.bnl.gov
> > > https://lists.bnl.gov/mailman/listinfo/star-fcv-l
> > > _______________________________________________
> > > Star-fcv-l mailing list
> > > Star-fcv-l AT lists.bnl.gov
> > > https://lists.bnl.gov/mailman/listinfo/star-fcv-l
> >
> >
> > Links:
> > ------
> > [1] https://drupal.star.bnl.gov/STAR/system/files/v2ratio.pdf
> > [2]
> https://drupal.star.bnl.gov/STAR/system/files/star_prelimilary_update.pdf